Observatory network
A planet-spanning detector array
No single detector can pinpoint where a gravitational wave came from. By comparing the arrival time and strength of a signal across detectors on different continents, scientists can triangulate its position on the sky.
LIGO Hanford
Hanford, Washington
LIGO Livingston
Livingston, Louisiana
Virgo
Cascina, near Pisa
KAGRA
Kamioka, Gifu
LIGO-India
Hingoli, Maharashtra
LIGO Hanford
United States
4 km dual-arm interferometer in the Pacific Northwest.
Operational
LIGO Livingston
United States
4 km interferometer ~3,000 km from Hanford.
Operational
Virgo
Italy
3 km European detector run by the EGO consortium.
Operational
KAGRA
Japan
Underground, cryogenic 3 km interferometer.
Operational
LIGO-India
India
Planned 4 km detector to widen the global network.
Under construction
Confirmation
Independent detectors rule out local noise — a real signal appears in multiple instruments.
Sky localization
Time differences between sites narrow down the patch of sky a wave came from.
Multi-messenger
Tighter localization helps telescopes point quickly to catch any accompanying light.